@inproceedings{1dac55c9959e4d028a4370bf12fdca5c,
title = "Population III supernova simulations of single and binary scenarios and reference to SN2006gy",
abstract = "We present stellar explosion simulations of low mass evolved and high mass polytrope Population III stars. The lower mass evolved single and binary models of 10 and 16M⊙ are presented in a separate work in these proceedings (Lawlor 2005). It is found that the accreted model retains a larger mass and has a larger radius leading to a brighter supernova than the evolved single stars. Polytropes are used as presupernova stars to investigate possible pair instability explosions of massive stars. SN 2006gy is a possible candidate for such an explosion (see Smith in these proceedings). We find upper limits based on the light curve analysis with M<50M⊙, R<355R ⊙, 56Nimass<5M⊙, and energy <100×1051 from the R-Band data. Theoretical supernova light curves are presented at different redshifts with our model that comes closest to fitting SN 2006gy.",
author = "Young, {T. R.} and Johnson, {T. A.} and Lawlor, {T. M.} and J. MacDonald",
year = "2008",
doi = "10.1063/1.2905550",
language = "English (US)",
isbn = "9780735405097",
series = "AIP Conference Proceedings",
pages = "233--237",
booktitle = "First Stars III",
note = "First Stars III ; Conference date: 15-07-2007 Through 20-07-2007",
}